References
Roberts, J. 2002. Does Dark Matter?. UK Dark Matter Collaboration. Department of Physics at Sheffield University. [Available:http://w ww.bbc.co.uk/science/space/deepspace/darkmatter/index.shtml]
Kneib, J.-P., Ellis, R. and Treu T. 2003. A Detailed Map of Dark Matter in a Galactic Cluster Reveals How Giant Cosmic Structures Formed. California Institute of Technology. [Available: http://pr.caltech.edu/media/Press_Releases/PR12 414.html]
Smith, N. 2003. The UK Dark Matter search at Boulby Mine. UK Dark Matter Collaboration. [Available: http://hepwww.rl.ac.uk/ukdmc/boulby/boulby.html]
Rees, M. and Natarajan, P. 2003. A Field Guide to the Invisible Universe. Discover. Vol.24 (12)42-9
Navigating the Deluge_ Dubai Floods and the Resilience of Dubai International...
SCNC 2002 - Dark Matter: Masses in Space that Go Undetected
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2. Blue line shows the slow decrease in orbital velocity. (After J.-C. Cuillandre, 2003)
3. Dark Matter Map, of galaxy cluster C10024+1654.(After Observatoire Midi-Pyrénées in France and Caltech.)
4. Efforts have been put to detect WIMPs using its unreactive nature – it should be able to pass through deep Earth, reaching detectors at 1100m deep, like this one in UK.
5. Neutrinos are ‘ghostly’ particles, which can only be detected using giant detectors with a heavy water basin, like this in Canada
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10. References Roberts, J. 2002. Does Dark Matter?. UK Dark Matter Collaboration . Department of Physics at Sheffield University. [Available:http://w ww.bbc.co.uk/science/space/deepspace/darkmatter/index.shtml] Kneib, J.-P., Ellis, R. and Treu T. 2003. A Detailed Map of Dark Matter in a Galactic Cluster Reveals How Giant Cosmic Structures Formed . California Institute of Technology. [Available: http://pr.caltech.edu/media/Press_Releases/PR12 414.html] Smith, N. 2003. The UK Dark Matter search at Boulby Mine . UK Dark Matter Collaboration. [Available: http://hepwww.rl.ac.uk/ukdmc/boulby/boulby.html ] Rees, M. and Natarajan, P. 2003. A Field Guide to the Invisible Universe. Discover. Vol.24 (12)42-9.
![Neutrinos are ‘ghostly’ particles, which can only be detected using giant detectors with a heavy water basin, like this in Canada Existence of Dark Matter: Its Evidences ,[object Object],Blue line shows the slow decrease in orbital velocity. (After J.-C. Cuillandre, 2003) ,[object Object],[object Object],[object Object],2. Gravitational Distortions ,[object Object],[object Object],[object Object],Dark Matter Map, of galaxy cluster C10024+1654.(After Observatoire Midi-Pyrénées in France and Caltech.) What are Dark Matters anyway? Characteristics ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],Likely Candidates Efforts have been put to detect WIMPs using its unreactive nature – it should be able to pass through deep Earth, reaching detectors at 1100m deep, like this one in UK. References Roberts, J. 2002. Does Dark Matter?. UK Dark Matter Collaboration . Department of Physics at Sheffield University. [Available:http://w ww.bbc.co.uk/science/space/deepspace/darkmatter/index.shtml] Kneib, J.-P., Ellis, R. and Treu T. 2003. A Detailed Map of Dark Matter in a Galactic Cluster Reveals How Giant Cosmic Structures Formed . California Institute of Technology. [Available: http://pr.caltech.edu/media/Press_Releases/PR12 414.html] Smith, N. 2003. The UK Dark Matter search at Boulby Mine . UK Dark Matter Collaboration. [Available: http://hepwww.rl.ac.uk/ukdmc/boulby/boulby.html ] Rees, M. and Natarajan, P. 2003. A Field Guide to the Invisible Universe. Discover. Vol.24 (12)42-9. Dark Matter: Masses in Space that Go Undetected By Chiu Hon Chim (2002315825) Detecting Dark Matter](https://image.slidesharecdn.com/scnc-2002-dark-matter-masses-in-space-that-go-undetected-26889/85/SCNC-2002-Dark-Matter-Masses-in-Space-that-Go-Undetected-1-320.jpg)
